MERLIN observations of relativistic ejections from GRS 1915+105
| Autor: | A. M. Stirling, T. W. B. Muxlow, Simon Garrington, Rob Fender, Ralph Spencer, Guy G. Pooley, E. B. Waltman, D. J. McKay |
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| Přispěvatelé: | High Energy Astrophys. & Astropart. Phys (API, FNWI) |
| Rok vydání: | 1999 |
| Předmět: |
Physics
Jet (fluid) Superluminal motion Proton Astrophysics::High Energy Astrophysical Phenomena Astrophysics (astro-ph) FOS: Physical sciences Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Electron Plasma Position angle Space and Planetary Science Ejecta Astrophysics::Galaxy Astrophysics MERLIN |
| Zdroj: | Monthly Notices of the Royal Astronomical Society, 304, 865-876. Oxford University Press |
| ISSN: | 1365-2966 0035-8711 |
| DOI: | 10.1046/j.1365-8711.1999.02364.x |
| Popis: | We present high resolution MERLIN radio images of multiple relativistic ejections from GRS 1915+105 in 1997 October / November. The observations were made at a time of complex radio behaviour, corresponding to multiple optically-thin outbursts and several days of rapid radio flux oscillations. The radio imaging resolved four major ejection events from the system. As previously reported from earlier VLA observations of the source, we observe apparent superluminal motions resulting from intrinsically relativistic motions of the ejecta. However, our measured proper motions are significantly greater than those observed on larger angular scales with the VLA. Under the assumption of an intrinsically symmetric ejection, we can place an upper limit on the distance to GRS 1915+105 of 11.2 +/- 0.8 kpc. Solutions for the velocities unambiguously require a higher intrinsic speed by about 0.1c than that derived from the earlier VLA observations, whilst the angle to the line-of-sight is not found to be significantly different. At a distance of 11 kpc, we obtain solutions of v = 0.98 (-0.05,+0.02)c and theta = 66 +/- 2 degrees. The jet also appears to be curved on a scale which corresponds to a period of around 7 days. We observe significant evolution of the linear polarisation of the approaching component, with large rotations in position angle and a general decrease in fractional polarisation. The power input into the formation of the jet is very large, >10^38 erg/s at 11 kpc for a pair plasma. If the plasma contains a cold proton for each electron, then the mass outflow rate, >10^18 g/sec is comparable to inflow rates previously derived from X-ray spectral fits. 14 pages, 7 figures. Accepted for publication in MNRAS |
| Databáze: | OpenAIRE |
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